Published 1979 | Version v1
Book

On the mass density distribution of the inner galaxy

Creators

  • 1. Kyoto Univ. (Japan). Dept. of Physics

Description

Based on current 2.4-micron observations of the Galaxy the author has proposed a specific model for the bulge component. This model is a concentric spheroid with an axial ratio of approximately 0.5. A constant mass-to-luminosity ratio M/Lsub(V) approximately 7.6 is assumed, which yields the relevant rotational velocity in the inner region; the absolute velocity is normalized to 250 km s-1. This value of M/Lsub(V) is likely to meet with giant-rich synthetic models for the nuclear bulge of M31. (Auth.)

Additional details

Publishing Information

Publisher
D. Reidel.
Imprint Place
Dordrecht, Netherlands
ISBN
90-277-1029-5
Imprint Title
The large-scale characteristics of the galaxy
Journal Page Range
p. 381-382.

Conference

Title
International Astronomical Union symposium no. 84 on the large-scale characteristics of the galaxy.
Dates
12 - 17 Jun 1978.
Place
College Park, MD, USA.

INIS

Country of Publication
Netherlands
Country of Input or Organization
Netherlands
INIS RN
11533382
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Numerical Data
Descriptors DEI
COMPILED DATA; GALAXY NUCLEI; GRAPHS; MILKY WAY; ROTATION; SPATIAL DISTRIBUTION; STARS; THEORETICAL DATA
Descriptors DEC
DATA; DATA FORMS; DISTRIBUTION; GALAXIES; INFORMATION; NUMERICAL DATA